Estimated redshift from machine learning (Ukwatta et al. 2016) - may take a few minutes to calcaulte
Image
Pre-slew 15-350 keV image (Event data; bkg subtracted)
# RAcent DECcent POSerr Theta Phi Peak Cts SNR Name
263.5279 -15.8204 0.3146 13.4 -3.6 0.7799 0.6 TRIG_01191994
------------------------------------------
Foreground time interval of the image:
0.000 183.020 (delta_t = 183.020 [sec])
Background time interval of the image:
Lightcurves
Notes:
- 1) All plots contain as much data as has been downloaded to date.
- 2) The mask-weighted light curves are using the flight position.
- 3) Multiple plots of different time binning/intervals are shown to cover all scenarios of short/long GRBs, rate/image triggers, and real/false positives.
- 4) For all the mask-weighted lightcurves, the y-axis units are counts/sec/det where a det is 0.4 x 0.4 = 0.16 sq cm.
- 5) The verticle lines correspond to following: green dotted lines are T50 interval, black dotted lines are T90 interval, blue solid line(s) is a spacecraft slew start time, and orange solid line(s) is a spacecraft slew end time.
- 6) Time of each bin is in the middle of the bin.
1 s binning
From T0-310 s to T0+310 s
From T100_start - 20 s to T100_end + 30 s
Full time interval
64 ms binning
Full time interval
From T100_start to T100_end
From T0-5 sec to T0+5 sec
16 ms binning
From T100_start-5 s to T100_start+5 s
8 ms binning
From T100_start-3 s to T100_start+3 s
2 ms binning
From T100_start-1 s to T100_start+1 s
SN=5 or 10 sec. binning (whichever binning is satisfied first)
SN=5 or 10 sec. binning (T < 200 sec)
Spectra
Notes:
- 1) The fitting includes the systematic errors.
- 2) For long bursts, a spectral fit of the pre-slew DRM will introduce some errors in both a spectral shape and a normalization if the PHA file contains a lot of the slew/post-slew time interval.
- 3) For fits to more complicated models (e.g. a power-law over a cutoff power-law), the BAT team has decided to require a chi-square improvement of more than 6 for each extra dof.
- 4) For short bursts (T90<1sec), the specrtum is also fit with Blackbody, OTTB, and Double Blackbody.
Time averaged spectrum fit using the pre-slew DRM
Power-law model
Time interval is from 0.000 sec. to 183.020 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.47814 ( -2.44594 -2.44594 )
Norm@50keV : 5.99756E-05 ( -6.01536e-05 0.000102897 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.88 using 59 PHA bins.
# Reduced chi-squared = 1.279 for 57 degrees of freedom
# Null hypothesis probability = 7.652879e-02
Photon flux (15-150 keV) in 183 sec: 1.16378E-02 ( -0.0116241 0.013777 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11233e-07 ( -1.08493e-07 1.66252e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 183.020 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.90421 ( 9.92102 11.999 )
Epeak [keV] : 24.1994 ( -8.55848 28.0321 )
Norm@50keV : 1.54784E+05 ( -171952 2.48486e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.32 using 59 PHA bins.
# Reduced chi-squared = 1.274 for 56 degrees of freedom
# Null hypothesis probability = 8.144351e-02
Photon flux (15-150 keV) in 183 sec: 1.33748E-02 1.32686E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.5274e-19 ( 0 0 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 183.020 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -13.793 -4.95633 )
beta : -9.81647 ( 9.81647 19.8056 )
Epeak [keV] : 23.4394 ( -11.1094 63.2623 )
Norm@50keV : 34.1270 ( -34.1878 2483.42 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.80 using 59 PHA bins.
# Reduced chi-squared = 1.305 for 55 degrees of freedom
# Null hypothesis probability = 6.367917e-02
Photon flux (15-150 keV) in 183 sec: 1.61413E-02 ( 6.98386 -0.0161413 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.79007 (-5.82372 -5.82372)
R^2/D10^2 : 5.78167E-02 (-0.0572128 -0.0572128)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.25 using 59 PHA bins.
# Reduced chi-squared = 1.268 for 57 degrees of freedom
# Null hypothesis probability = 8.398643e-02
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.470e-08 3.482e-08
25- 50 4.121e-08 3.298e-08
50-150 3.254e-09 5.871e-09
15-150 8.916e-08 6.119e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 27.8784 (-27.8784 -27.8784)
Norm : 0.106212 (-0.106212 -0.106212)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.803e-08 3.015e-08
25- 50 4.167e-08 3.588e-08
50-150 2.068e-08 3.075e-08
15-150 1.004e-07 8.971e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.57247 (-5.56467 -5.56467)
R1^2/D10^2 : 6.35257E-02 (-0.0641363 -0.0641363)
kT2 [keV] : 18.6114 (-18.5557 -18.5557)
R2^2/D10^2 : 1.03188E-04 (-0.000105529 -0.000105529)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.409e-08 3.955e-08
25- 50 4.231e-08 5.459e-08
50-150 1.798e-08 6.548e-09
15-150 1.044e-07 1.251e-07
Peak spectrum fit
Power-law model
Time interval is from 0.000 sec. to 183.020 sec.
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.47814 ( -2.44594 -2.44594 )
Norm@50keV : 5.99756E-05 ( -6.01536e-05 0.000102897 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.88 using 59 PHA bins.
# Reduced chi-squared = 1.279 for 57 degrees of freedom
# Null hypothesis probability = 7.652879e-02
Photon flux (15-150 keV) in 183 sec: 1.16378E-02 ( -0.0116241 0.013777 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11233e-07 ( -1.08493e-07 1.66252e-07 ) ergs/cm2
Cutoff power-law model
Time interval is from 0.000 sec. to 183.020 sec.
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.90421 ( 9.92102 11.999 )
Epeak [keV] : 24.1994 ( -8.55848 28.0321 )
Norm@50keV : 1.54784E+05 ( -171952 2.48486e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.32 using 59 PHA bins.
# Reduced chi-squared = 1.274 for 56 degrees of freedom
# Null hypothesis probability = 8.144351e-02
Photon flux (15-150 keV) in 183 sec: 1.33748E-02 1.32686E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.5274e-19 ( 0 0 ) ergs/cm2
Band function
Time interval is from 0.000 sec. to 183.020 sec.
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -14.6479 -4.95633 )
beta : -9.81647 ( 9.81647 19.8056 )
Epeak [keV] : 23.4394 ( -10.9552 61.6539 )
Norm@50keV : 34.1270 ( -34.1878 2483.42 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.80 using 59 PHA bins.
# Reduced chi-squared = 1.305 for 55 degrees of freedom
# Null hypothesis probability = 6.367917e-02
Photon flux (15-150 keV) in 183 sec: 1.61413E-02 ( 6.98386 -0.0161413 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
Single BB
XSPEC: quit
Spectral model blackbody:
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 5.79007 (-5.82372 -5.82372)
R^2/D10^2 : 5.78167E-02 (-0.0572128 -0.0572128)
(R is the radius in km and D10 is the distance to the source in units of 10 kpc)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.470e-08 3.289e-08
25- 50 4.121e-08 2.966e-08
50-150 3.254e-09 4.903e-09
15-150 8.916e-08 6.524e-08
Thermal bremsstrahlung (OTTB)
XSPEC12>exit
XSPEC: quit
Spectral model: thermal bremsstrahlung
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT [keV] : 27.8784 (-27.8784 -27.8784)
Norm : 0.106212 (-0.106212 -0.106212)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 3.803e-08 3.072e-08
25- 50 4.167e-08 3.650e-08
50-150 2.068e-08 2.546e-08
15-150 1.004e-07 9.571e-08
Double BB
XSPEC12>exit
XSPEC: quit
Spectral model: bbodyrad<1> + bbodyrad<2>
------------------------------------------------------------
Parameters : value Lower 90% Upper 90%
kT1 [keV] : 5.57247 (-5.56467 -5.56467)
R1^2/D10^2 : 6.35257E-02 (-0.0641363 -0.0641363)
kT2 [keV] : 18.6114 (-18.5557 -18.5557)
R2^2/D10^2 : 1.03188E-04 (-0.000105529 -0.000105529)
------------------------------------------------------------
Reduced chi-squared =
Energy Fluence 90% Error
[keV] [erg/cm2] [erg/cm2]
15- 25 4.409e-08 3.837e-08
25- 50 4.231e-08 4.458e-08
50-150 1.798e-08 2.081e-08
15-150 1.044e-07 1.310e-07
Pre-slew spectrum (Pre-slew PHA with pre-slew DRM)
Power-law model
Spectral model in power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: 2.47814 ( -2.44594 -2.44594 )
Norm@50keV : 5.99756E-05 ( -6.01536e-05 0.000102897 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 72.88 using 59 PHA bins.
# Reduced chi-squared = 1.279 for 57 degrees of freedom
# Null hypothesis probability = 7.652879e-02
Photon flux (15-150 keV) in 183 sec: 1.16378E-02 ( -0.0116241 0.013777 ) ph/cm2/s
Energy fluence (15-150 keV) : 1.11233e-07 ( -1.08493e-07 1.66252e-07 ) ergs/cm2
Cutoff power-law model
Spectral model in the cutoff power-law:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
Photon index: -9.90421 ( 9.92102 11.999 )
Epeak [keV] : 24.1994 ( -8.55848 28.0321 )
Norm@50keV : 1.54784E+05 ( -171952 2.48486e+07 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.32 using 59 PHA bins.
# Reduced chi-squared = 1.274 for 56 degrees of freedom
# Null hypothesis probability = 8.144351e-02
Photon flux (15-150 keV) in 183 sec: 1.33748E-02 1.32686E-02 ( ) ph/cm2/s
Energy fluence (15-150 keV) : 2.5274e-19 ( 0 0 ) ergs/cm2
Band function
Spectral model in the Band function:
------------------------------------------------------------
Parameters : value lower 90% higher 90%
alpha : 5.00000 ( -14.7729 -4.95633 )
beta : -9.81647 ( 9.81647 19.8056 )
Epeak [keV] : 23.4394 ( -11.136 63.3143 )
Norm@50keV : 34.1270 ( -34.1878 2483.42 )
------------------------------------------------------------
#Fit statistic : Chi-Squared = 71.80 using 59 PHA bins.
# Reduced chi-squared = 1.305 for 55 degrees of freedom
# Null hypothesis probability = 6.367917e-02
Photon flux (15-150 keV) in 183 sec: 1.61413E-02 ( 6.98386 -0.0161413 ) ph/cm2/s
Energy fluence (15-150 keV) : 0 ( 0 0 ) ergs/cm2
S(25-50 keV) vs. S(50-100 keV) plot
S(25-50 keV) = 3.66e-08
S(50-100 keV) = 2.72e-08
T90 vs. Hardness ratio plot
T90 = 808 sec.
Hardness ratio (energy fluence ratio) = 0.743169
Color vs. Color plot
Count Ratio (25-50 keV) / (15-25 keV) = 0.261845
Count Ratio (50-100 keV) / (15-25 keV) = 0.132892
Mask shadow pattern
IMX = 2.382836336680777E-01, IMY = 1.485840068430309E-02
TIME vs. PHA plot around the trigger time
TIME vs. DetID plot around the trigger time
100 us light curve (15-350 keV)
Spacecraft aspect plot
Bright source in the pre-burst/pre-slew/post-slew images
Pre-burst image of 15-350 keV band
Time interval of the image:
Pre-slew background subtracted image of 15-350 keV band
Time interval of the image:
0.000000 183.020000
# RAcent DECcent POSerr Theta Phi PeakCts SNR AngSep Name
# [deg] [deg] ['] [deg] [deg] [']
244.9725 -15.6530 0.6 23.8 -52.2 11.2375 18.7 0.9 Sco X-1
255.9342 -37.8656 1.5 12.4 -130.0 3.4871 7.6 2.8 4U 1700-377
256.5804 -36.3900 5.4 11.1 -126.2 1.0399 2.1 7.3 GX 349+2
263.0672 -24.8014 5.5 5.1 -27.6 -1.0471 -2.1 4.6 GX 1+4
264.9250 -44.3325 8.0 15.4 -167.8 -0.7114 -1.5 10.5 4U 1735-44
268.3559 -1.6047 5.8 27.5 12.6 1.2854 2.0 9.2 SW J1753.5-0127
270.4038 -25.1027 6.4 5.3 52.0 0.8939 1.8 6.7 GX 5-1
270.1096 -25.6216 0.0 4.7 53.8 -0.7470 -1.5 12.7 GRS 1758-258
273.9120 -13.9022 4.1 16.6 34.7 1.5221 2.8 9.7 GX 17+2
276.0691 -30.3638 4.6 8.5 109.9 1.2012 2.5 7.5 H1820-303
284.9273 -25.0999 5.5 17.0 89.4 1.2860 2.1 12.3 HT1900.1-2455
288.7771 10.9716 11.5 45.4 40.0 -1.3489 -1.0 2.0 GRS 1915+105
263.1638 -33.7886 30.0 5.5 -142.9 0.1890 0.4 9.1 GX 354-0
276.4706 -33.7954 2.3 9.9 130.0 2.3791 5.0 ------ UNKNOWN
261.9332 -16.2037 0.2 13.4 -10.4 26.2975 53.2 ------ UNKNOWN
Post-slew image of 15-350 keV band
Time interval of the image:
Plot creation:
Fri Sep 15 03:52:59 EDT 2023